\begin{table}%t1
%\centering
\par
\caption{\label{tab1}Results from SED modelling.}
 \begin{tabular}{lccccccccccccc}
\hline\hline
\noalign{\smallskip}
Name           &  $M_*$      &   $R_*$      &   $T_*$       &  ${\dot{M}}_{\rm env}$     &  $M_{\rm disk}$  &  ${\dot{M}}_{\rm disk}$   &  Rout$_{\rm env}$    &  Rout$_{\rm disk}$    &  Rin$_{\rm env}$    \\
               &  \msun      &  log~(\rsun)  &  log~($K$)    &  log~(\msun yr$^{-1}$)  &  log(\msun)  &  log~(\msun yr$^{-1}$) &  AU              & AU	         &  $R$sub\tablefootmark{*}          \\
\hline   
I20293-IRS~1  & 6.8~$\pm$~0.9 & 1.3~$\pm$~0.3  & 3.8~$\pm$~0.2   & --3.9~$\pm$~1.2 	   & --2.2~$\pm$~1.3 & --7.6~$\pm$~1.5	  & 37~682~$\pm$~2      & 117~$\pm$~3         & 1~$\pm$~1	   \\
I05358-IRS~1  & 6.8~$\pm$~0.3 & 1.2~$\pm$~0.2  & 3.8~$\pm$~0.1   & --4.8~$\pm$~0.8 	   & --2.1~$\pm$~0.5 & --7.5~$\pm$~0.7	  & 24~731~$\pm$~2      & 101~$\pm$~2         & 4~$\pm$~1	    \\
\hline 
\end{tabular}
\tablefoot{\tablefoottext{*}{$R$sub is the dust destruction radius, common to both the disk and envelope. See \citet{rob06} for details.}}
\end{table}